Ultra-strong MgII absorbers at z=0.4-1.7 are mostly hosted by low-mass, star-forming galaxies, with the absorbing gas preferentially located along the disk and wind axes, and many absorbers lacking a detected host.
I., Grogin, N., & Koekemoer, A
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Baryonic Ecosystem in Galaxies (BEINGMgII). Host Galaxies of Ultra-strong MgII Absorbers in Subaru Hyper Suprime-Cam Survey
Ultra-strong MgII absorbers at z=0.4-1.7 are mostly hosted by low-mass, star-forming galaxies, with the absorbing gas preferentially located along the disk and wind axes, and many absorbers lacking a detected host.